SDO HMI 2011-09-05 13:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.74 | 87.06 | 16.37 | 57.67 | -19.55 | 258.68 | 32.52 | 229.54 | 0.6679 | 281.5 | 365.5 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.52 | 0.00 | 1.08 | -22.11 | 261.82 | 35.66 | 229.08 | 0.7170 | 590.0 | 441.1 | |
| 0.00 | 1.16 | 0.00 | 0.83 | -23.59 | 261.75 | 35.58 | 227.37 | 0.7271 | 518.0 | 407.6 | |
| 0.00 | 2.14 | 0.00 | 1.51 | -23.07 | 260.82 | 34.66 | 227.23 | 0.7150 | 577.0 | 447.3 | |
| 2.05 | 3.48 | 1.38 | 2.34 | -19.97 | 259.17 | 33.01 | 229.46 | 0.6760 | 442.0 | 377.9 | |
| 16.52 | 58.14 | 11.00 | 38.53 | -19.51 | 258.95 | 32.79 | 229.82 | 0.6704 | 893.5 | 539.3 | |
| 0.00 | 0.54 | 0.00 | 0.36 | -20.14 | 258.67 | 32.51 | 228.84 | 0.6725 | 414.0 | 370.2 | |
| 2.41 | 7.86 | 1.57 | 5.14 | -18.44 | 258.03 | 31.87 | 230.34 | 0.6529 | -593.7 | 135.5 | |
| 1.88 | 3.30 | 1.22 | 2.15 | -18.93 | 257.38 | 31.22 | 229.17 | 0.6503 | -521.3 | -528.1 | |
| 0.00 | 0.89 | 0.00 | 0.61 | -22.70 | 258.24 | 32.07 | 225.51 | 0.6890 | 608.0 | 549.1 | |
| 0.00 | 1.16 | 0.00 | 0.75 | -18.79 | 257.28 | 31.12 | 229.25 | 0.6481 | -677.0 | -550.8 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -18.68 | 256.63 | 30.46 | 228.80 | 0.6406 | -542.0 | -339.5 | |
| 1.88 | 2.23 | 1.20 | 1.43 | -18.39 | 256.23 | 30.07 | 228.80 | 0.6342 | -718.5 | -581.0 | |
| 0.00 | 1.61 | 0.00 | 1.01 | -17.53 | 255.42 | 29.25 | 229.11 | 0.6187 | -649.0 | -555.6 | |
| 0.00 | 1.43 | 0.00 | 0.91 | -19.51 | 255.42 | 29.26 | 226.67 | 0.6357 | -737.0 | -580.8 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -17.59 | 254.20 | 28.03 | 227.84 | 0.6066 | -688.0 | -486.7 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |